SED fitting results for "The initial-to-final mass relation of white dwarfs in intermediate-separation binaries"

SED Fitting Results. Both $\chi^2_\text{IR}$ and $\chi^2_\text{opt}$ are calculated using both optical and IR data, and normalized by the number of degrees of freedom ($N_\text{IR}+N_\text{opt} - 2$). However, $\chi^2_\text{opt}$ is calculated using the model fit to optical data only. Candidates 101, 140, 160, 192, 194, 282 are suspected of showing IR excess, and therefore are not given a full optical+IR fit. $T_\text{eff,2}$ values are obtained from the full binary fit for candidates with UV excess. \label{tab:sed_results}